Volcanism is a fundamental process in the geological evolution of the Moon, providing clues
to the composition and structure of the mantle, the location and duration of interior melting …

The Moon is a unique body in our Solar System that allows us to groundtruth remotesensing
data (eg, crater size–frequency distributions, or CSFDs, crater/rock degradation rates …

We utilize a theoretical analysis of the generation, ascent, intrusion and eruption of basaltic
magma on the Moon to develop new insights into magma source depths, supply processes …

Apollo and Luna landing site samples, regional stratigraphic relationships, and crater
degradation and size-frequency distribution data for units largely defined prior to the end of …

We model the ascent and eruption of lunar mare basalt magmas with new data on crustal
thickness and density (GRAIL), magma properties, and surface topography, morphology and …

We report the surface exploration by the lunar rover Yutu that landed on the young lava flow
in the northeastern part of the Mare Imbrium, which is the largest basin on the nearside of …

Unraveling the timing and duration of mare volcanism on the Moon is essential for
understanding its thermal evolution. The end of mare volcanism is poorly constrained …

The chemical compositions of relatively young mare lava flows have implications for the late
volcanism on the Moon. Here we report the composition of soil along the rim of a 450-m …

Moon Mineralogy Mapper (M3) image and spectral reflectance data are combined to
analyze mare basalt units in and adjacent to the Orientale multiring impact basin. Models …

The last major phases of lunar volcanism produced spectrally unique high‐titanium basalts
on the western nearside of the Moon. The Moon Mineralogy Mapper (M3) on Chandrayaan …